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Self‐Similar Evolution of Gravitational Clustering. II. N‐Body Simulations of the n = −2 Spectrum

  • Authors: Bhuvnesh Jain and Edmund Bertschinger

Jain & Bertschinger 1998 The Astrophysical Journal 509 517.

  • Provider: AAS Journals

Caption: Fig. 14.

Characteristic scales from the amplitude for n = 0. For n = 0 the scaling kc vs. a is shown using the mean amplitude. Again, as in Fig. 13, the standard self‐similar scaling is recovered.

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